Non-Hamiltonian Kelvin wave generation on vortices in Bose-Einstein condensates
Scott A. Strong, Lincoln D. Carr

TL;DR
This paper introduces a non-Hamiltonian generalization of the local induction approximation for vortex lines in Bose-Einstein condensates, revealing mechanisms for Kelvin wave generation and propagation through curvature reconfiguration.
Contribution
It derives a generalized vortex filament model that incorporates non-Hamiltonian effects, enabling Kelvin wave motion in quantum turbulence simulations.
Findings
Reveals non-Hamiltonian evolution leads to Kelvin wave propagation.
Derives a modified nonlinear Schrödinger equation for vortex curvature.
Simulations demonstrate dispersive and deforming curvature profiles.
Abstract
Ultra-cold quantum turbulence is expected to decay through a cascade of Kelvin waves. These helical excitations couple vorticity to the quantum fluid causing long wavelength phonon fluctuations in a Bose-Einstein condensate. This interaction is hypothesized to be the route to relaxation for turbulent tangles in quantum hydrodynamics. The local induction approximation is the lowest order approximation to the Biot-Savart velocity field induced by a vortex line and, because of its integrability, is thought to prohibit energy transfer by Kelvin waves. Using the Biot-Savart description, we derive a generalization to the local induction approximation which predicts that regions of large curvature can reconfigure themselves as Kelvin wave packets. While this generalization preserves the arclength metric, a quantity conserved under the Eulerian flow of vortex lines, it also introduces a…
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Taxonomy
TopicsFluid Dynamics and Turbulent Flows · Quantum, superfluid, helium dynamics · Cold Atom Physics and Bose-Einstein Condensates
